Fast Gravitational Wave Radiometry using Data Folding
Anirban Ain, Prathamesh Dalvi, Sanjit Mitra

TL;DR
This paper introduces a data folding technique for gravitational wave radiometry that significantly reduces computational costs and data volume, enabling more efficient and flexible analysis of stochastic gravitational wave backgrounds.
Contribution
The authors develop a novel data folding method for GW radiometry that preserves analysis precision while drastically reducing computational and storage requirements.
Findings
Orders of magnitude reduction in computation time.
Data volume decreased to a few gigabytes.
Validated on LIGO data with consistent results.
Abstract
Gravitational Waves (GWs) from the early universe and unresolved astrophysical sources are expected to create a stochastic GW background (SGWB). The GW radiometer algorithm is well suited to probe such a background using data from ground based laser interferometric detectors. Radiometer analysis can be performed in different bases, e.g., isotropic, pixel or spherical harmonic. Each of these analyses possesses a common temporal symmetry which we exploit here to fold the whole dataset for every detector pair, typically a few hundred to a thousand days of data, to only one sidereal day, without any compromise in precision. We develop the algebra and a software pipeline needed to fold data, accounting for the effect of overlapping windows and non-stationary noise. We implement this on LIGO's fifth science run data and validate it by performing a standard anisotropic SGWB search on both…
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